No sign of gravitational lensing in the cosmic microwave background

by Ron Samec

Gravitational lensing is a gravitational-optical effect whereby a background object
like a distant quasar is magnified, distorted and brightened by a foreground galaxy.
It is one of the consequences of general relativity and is so well understood that
it now appears in standard optics text books. Objects that are too far to be seen
are ‘focused’ by an intervening concentration of matter and bought into
view to the earth based astronomer. One of the most interesting photos of the effects
of gravitational lensing is shown in the HST image of Abell 2218 by Andrew Fruchter1 (Space telescope Science Institute)
et al., with the WFPC2 camera,2
on the Hubble Space Telescope (NASA) (see illustration 1.).

Image by Andrew Fruchter (STScI) et al., WFPC2, HST, NASA

It is alleged that the cluster of galaxies Abell 2218, distorts and magnifies light
from galaxies behind it.

In this image, the cluster of galaxies, Abell 2218 is distorting and magnifying
light from galaxies behind it. They appear as ring arcs of faint light. This cluster
is about three million light years distant. One of the most distant objects discovered
is a galaxy that was detected at 5.6 GLY (5.6 billion light years) distant using
Abell 2218 as a ‘lens’.

It is alleged that the farthest known background radiation sources in the cosmos
are what we call the cosmic microwave background, or the CMB. This was supposed
to be formed when photons were released in the big bang decoupling event when the
universe became ‘transparent’. The temperature this occurred at was
about 3000 K, when normal hydrogen gas formed, supposedly some 380,000 years after
the big bang. The space had spread by a factor of 1000, dropping the observable
blackbody temperature of this event to 3 K and forming this all pervasive background
to the universe. The background gives almost a perfectly smooth black body spectrum
of 2.725 K with very tiny fluctuations in the pattern on the 70 μK level. These
‘bumps’ or patterns in the CMB are supposedly the ‘seeds’
from which the galaxies formed. Why is it so smooth? Alan Guth ‘solved’
this puzzle by postulating that the universe was originally a very tiny entity in
thermal equilibrium. It ‘inflated’ from about 10–35
to 10–24 seconds after the big bang at many times the speed of
light and then it began its ordinary expansion.

The largest foreground concentrations of matter in the universe, which cause appreciable
gravitational lensing, are galactic clusters. The WMAP (Wilkinson Microwave Anisotropy
Probe) recently imaged the CMB of the full sky to a high resolution. One would expect
to see gravitational lensing distortions caused by the foreground galactic clusters
in the CMB ‘acoustic’ patterns. Lieu and Mitaz3 in their recent article have shown mathematically
that the expected distortions in the CMB are absent!

If the CMB is not of cosmological origin, all the ad hoc ideas that have been added
to support the big bang theory (like inflation) fall apart.

‘But you don’t see this fluctuation’, said Lieu. ‘There
appear to be no lensing effects whatsoever. This lack of variation is a serious
problem.’4

This is a major blow to the big bang theory where the existence of the CMB is the
main evidence for its occurrence.

This may mean that the CMB is not ‘cosmological’ at all, but rather
a ‘local’ effect, possibly like that envisioned by Hoyle and Wickramasinghe
and by Hartnett.5,6 They showed that a homogeneous cloud mixture of
carbon/silicate dust and iron or carbon whiskers could produce such a background
radiation. If the CMB is not of cosmological origin, all the ad hoc ideas
that have been added to support the big bang theory (like inflation) fall apart.

Thus the CMB may not be the ‘whimper’ of the big bang, but just a rather
homogeneous but dirty expulsion of a nearby supernova.7

However, it is hard, in my thinking, to conceive that any
natural manifestation could produce so smooth a pattern. Return to
text.

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